Diffuse Matter in the Galaxy - An International Conference

On behalf of the Scientific Organizing committee ofthe international meeting, Diffuse Matter in the Galaxy: Observations Confront Theory, we seek NSF funding for partial conference travel support of students and early career scientists at U.S. institutions. An important objective of the meeting is to facilitate close interactions among established researchers engaged in the study of the interstellar medium (ISM) and their more junior colleagues. These younger investigators will ensure the future development of this fundamental research field. Financial assistance for travel expenses of early career researchers will assure that this objective can be met. We also seek partial travel support for a very limited number of senior participants. Intellectual Merit: The theoretical concept ofthe ISM in the Milky Way as a multi-component environment is useful because it allows calculations to be made of the ionization structure, the temperature structure and the energy balance that characterizes this material. These physical quantities, in turn, can be related to the presumed sources of energy input to the ISM -luminous stars, stellar winds and supernovae. Finally, one can check for consistency with observation and assess the need for an increasing sophistication of the theoretical models. Recent observations of the ISM, using a wide variety of new techniques, have underscored the extreme diversity of this medium. A significant mass fraction ofthe ISM exists as cold gas with temperatures less than 100 K, a comparable mass fraction (but much larger volume fraction) exists as warm gas, and a large volume is filled with very dilute gas having temperatures of hundreds of thousands or even millions of K. The nature of each of these regions is being probed by specially-designed telescopes and detectors. Moreover, each is being studied theoretically using the physics relevant to the gas densities and temperatures observed. But less progress has been made in understanding the connections that exist among these phases of the ISM and the processes that transform one phase into another. Understanding these connections is a primary goal of the meeting Diffuse Matter in the Galaxy: Observations Confront Theory. Broader Impact: As mentioned above, an important objective of the meeting is to bring together established ISM researchers and their junior colleagues. Interactions between these two groups will stimulate future research collaborations, formal or informal. And interactions like these are essential if the field ofISM research is to remain active and vital in the future. Obviously, this goal cannot be met unless a substantial number of younger researchers attend the meeting. A second objective of this meeting is to create a conference publication oflasting value. We envision a publication consisting of at least seven comprehensive reviews of the conference session topics outlined in this proposal. We believe such a publication will be suitable as a basic textbook for introductory graduate courses in observations and theory of the ISM. Ifwe are successful in this latter objective, the broader impact of the conference will be spread to future generations of students, students who we hope will be inspired by our work. However, we do not seek NSF funding for such a publication.